High-resolution 21-cm observations of low-column density gas clumps in the Milky Way halo

Astronomy and Astrophysics

Volumn 503, Issue 2, 2009, Pages 483-493

  Ben Bekhti, N ^a   Richter, P ^b   Winkel, B ^a   Kenn, F ^a   Westmeier, T ^c  

^a UNIVERSITY OF BONN   (Germany)

^b UNIVERSITY OF POTSDAM   (Germany)

^c CSIRO   (Australia)

Author keywords

Galaxies: Halos; Galaxy: Halo; ISM: Structure; Quasars: Absorption lines

Indexed keywords

ALL-SKY SURVEY; ANGULAR SCALE; ANGULAR SIZES; COLUMN DENSITY; GALAXIES: HALOS; GALAXY: HALO; HIGH RESOLUTION; HIGH VELOCITY; INTERFEROMETRIC DATA; ISM: STRUCTURE; KINETIC TEMPERATURES; LINES-OF-SIGHT; LOW-COLUMN DENSITY GAS CLUMPS; LOW-MASS; MAGELLANIC STREAM; MILKY WAYS; NEUTRAL GAS; OPTICAL ABSORPTION; OPTICAL SPECTRA; QUASAR SPECTRA; QUASARS:ABSORPTION LINES; RADIAL VELOCITY; THEORETICAL MODELS; THERMAL GAS; UPPER LIMITS; VERY LARGE ARRAYS;

CLOUDS; GALAXIES; GAS ABSORPTION; GASES; SODIUM; TELESCOPES; VELOCITY;

DENSITY OF GASES;

EID: 77957844950     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811259     Document Type: Article

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